We complement these data with the proper motions, photometry, and extinction from the EDR3 Gaia catalogue [1]}. The cross-match between every Gaia-ESO spectrum and Gaia ED3 catalogue was performed on grounds of angular position within a \(1.0\)  arcsec tolerance (cone search). Distances and their uncertainties were adopted from [2]}. The spatial distribution of the sample is shown in Fig. REF . Most of these objects are confined closer to the plane with altitudes of up to \(~2\)  kpc and they probe a range of Galactocentric radii from \(\sim 5\)  to 12 kpc. The 3D space velocitiesIn this work, we use galactocentric cylindrical coordinate system. So that V\(_{\rm r}\) , V\(_{\phi }\) , V\(_z\)  are the components of the full 3D space velocity pointing towards Galactic center R, in the direction of rotation \(\phi \) , and vertically relative to the disc mid-plane, respectively. for the sample are calculated using the Python package 'astropy' [3]}, [4]}. The accuracy of the astrometric information is high enough to yield the velocities with the uncertainty of \(\lesssim 5\)  kms\(^{-1}\) .
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